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Table 1

Measured and derived properties.

Galaxy Position Redshift Obs. CO SCOΔV W CO Flaga Ref. CO log(M) Metallicityb
RA Dec Transition Jy km s-1 km s-1 109 K km s-1pc2 log (M) 12+log (O/H)

PEPJ123712+621753 12 37 12.15 62 17 53.95 1.249 2−1 0.15 ± 0.04 409 ± 170 1 4.2 ± 1.1 This work 10.62 8.73
PEPJ123709+621507 12 37 09.13 62 15 07.92 1.224 2−1 0.28 ± 0.06 231 ± 90 2 7.5 ± 1.6 This work 10.36 8.67
PEPJ123759+621732 12 37 59.47 62 17 32.86 1.084 2−1 0.44 ± 0.11 406 ± 115 1 9.3 ± 2.3 This work 10.58 8.72
PEPJ123721+621346 12 37 21.45 62 13 46.06 1.021 2−1 0.39 ± 0.13 236 ± 160 2 7.3 ± 2.4 This work 10.53 8.71
PEPJ123615+621008 12 36 15.19 62 10 08.65 1.027 2−1  <0.42 ... 3 7.9 ± 1.5 This work 10.90 8.78
PEPJ123634+620627 12 36 34.50 62 06 27.94 1.215 2−1  <0.27 ... 3 7.1 ± 1.3 This work 11.06 8.80
PEPJ123633+621005 12 36 33.65 62 10 05.77 1.016 2−1 0.78 ± 0.19 393 ± 120 2 14.4 ± 3.5 This work 10.97 8.79
PEPJ123646+621141 12 36 46.18 62 11 41.99 1.016 2−1 0.40 ± 0.09 157 ± 60 1 7.4 ± 1.6 This work 11.06 8.80
PEPJ123750+621600 12 37 50.89 62 16 00.69 1.170 2−1 0.53 ± 0.08 649 ± 110 1 13.0 ± 1.9 This work 11.31 8.83
HDF169 12 36 34.53 62 12 40.92 1.224 2−1 3.45 ± 0.93 560 ... 92.3 ± 24.9 Frayer+2008 10.63 8.73
BzK-4171 12 36 26.52 62 08 35.30 1.465 2−1 0.65 ± 0.08 530 ... 24.6 ± 3.0 Daddi+2010 10.72 8.75
BzK-21000 12 37 10.64 62 22 34.17 1.523 2−1 0.64 ± 0.07 444 ... 26.0 ± 2.8 Daddi+2010 10.99 8.75
BzK-16000 12 36 30.09 62 14 27.96 1.522 2−1 0.46 ± 0.05 194 ... 18.7 ± 2.0 Daddi+2010 10.98 8.75
BzK-17999 12 37 51.82 62 15 20.11 1.414 2−1 0.57 ± 0.06 440 ... 20.1 ± 2.1 Daddi+2010 11.18 8.82
BzK-12591 12 37 41.37 62 12 51.18 1.600 2−1 0.84 ± 0.16 600 ... 37.5 ± 7.1 Daddi+2010 11.32 8.79
HDF242 12 37 07.20 62 14 08.08 2.490 1−0 0.21 ± 0.03 850 ... 62.5 ± 8.9 Ivison+2011 11.41 8.80
GN20 12 37 11.87 62 22 12.46 4.050 2−1 0.64 ± 0.16 670 ... 142.1 ± 35.5 Carilli+2010 11.40 8.80

Notes. 

(a)

Significance of our PdBI detections: 1) secure detection; 2) tentative detection; 3) upper limit.

(b)

Metallicity are estimated using the mass-metallicity relation and converted into the Denicoló et al. (2002) system.

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